CM2 Meteorites

carbonaceous group · 416 meteorites

CM2 carbonaceous chondrites are carbon-rich, hydrated meteorites. They contain up to 3% carbon, amino acids, and water-bearing minerals. Important for understanding organic chemistry in the early solar system.

Sort by: Mass Name Year Country
Name Mass
MacAlpine Hills 02701 10.1 g
Yamato 980094 10.1 g
Dhofar 1277 10.0 g
Pecora Escarpment 02050 9.8 g
MacKay Glacier 05229 9.7 g
Yamato 980183 9.5 g
Yamato 86690 9.5 g
Elephant Moraine 96012 9.4 g
Yamato 86039 9.3 g
Meteorite Hills 01076 9.2 g
Meteorite Hills 00632 9.1 g
Queen Alexandra Range 93017 8.8 g
LaPaz Icefield 031371 8.8 g
Queen Alexandra Range 99443 8.7 g
Elephant Moraine 83224 8.6 g
Yamato 980086 8.4 g
Allan Hills 85004 8.4 g
Dominion Range 08015 8.4 g
Dominion Range 08010 8.3 g
Yamato 980239 8.2 g
Yamato 794083 8.2 g
Yamato 794074 8.1 g
Yamato 75293 8.1 g
LaPaz Icefield 031043 8.1 g
Reckling Peak 92402 8.0 g
Miller Range 090443 7.9 g
Allan Hills 84032 7.9 g
LaPaz Icefield 02302 7.9 g
Reckling Peak 92400 7.8 g
Miller Range 07670 7.7 g
Yamato 982069 7.6 g
Yamato 793564 7.5 g
Miller Range 07702 7.4 g
Yamato 794077 7.4 g
Graves Nunataks 06131 7.3 g
Lewis Cliff 88002 7.2 g
LaPaz Icefield 04754 7.2 g
MacAlpine Hills 02606 7.2 g
Meteorite Hills 001012 7.1 g
Queen Alexandra Range 94582 7.1 g
LaPaz Icefield 04565 7.1 g
Reckling Peak 92401 7.0 g
Allan Hills 88052 7.0 g
LaPaz Icefield 031299 6.9 g
Miller Range 090532 6.9 g
LaPaz Icefield 02348 6.9 g
Miller Range 11040 6.8 g
Yamato 790123 6.8 g
Yamato 981288 6.7 g
Roberts Massif 03523 6.7 g

Related Classifications